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http://hdl.handle.net/2248/2223| Title: | Flat Spectrum Gamma Ray Burst Afterglows |
| Authors: | Bhattacharya, D |
| Keywords: | Gamma Ray Bursts Afterglow Radiation mechanism Theory |
| Issue Date: | 2001 |
| Publisher: | Astronomical Society of India |
| Citation: | BASI, Vol. 29, No. 2, pp. 107 - 114 |
| Abstract: | Temporal behaviour of GRB afterglow light curve is derived for the case where the electron energy distribution is relatively hard, with the power-law index p lying between 1.0 and 2.0. It is shown that the expected behaviour will be the same as that for p > 2.0 if the upper cutoff in the electron energy distribution evolves in direct proportion to the bulk Lorentz factor of the blast wave. |
| URI: | http://hdl.handle.net/2248/2223 |
| Appears in Collections: | BASI Publications |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| bhattac.pdf | 604.59 kB | Adobe PDF |  View/Open |
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